<?xml version="1.0" encoding="utf-8"?>
<!-- Produced with astropy.io.votable version 0.2.dev2731
     http://www.astropy.org/ -->
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 <DESCRIPTION>
  VOTable generated from the original AAS Journal Machine Readable
  Table
 </DESCRIPTION>
 <COOSYS ID="J2000" epoch="J2000." equinox="J2000." system="eq_FK5"/>
 <RESOURCE ID="aj285677t2_votable" type="results">
  <DESCRIPTION>
   Intrinsically Red Sources observed by Spitzer in the Galactic Mid-
   Plane  (Robitaille T.P. et al.)
  </DESCRIPTION>
  <LINK href="http://dx.doi.org/10.1088/0004-6256/136/6/2413"/>
  <TABLE nrows="18949">
   <DESCRIPTION>
    Final red source catalog
   </DESCRIPTION>
   <FIELD ID="col1" arraysize="25" datatype="char" name="Name" ucd="meta.id;meta.main" unit="---">
    <DESCRIPTION>
     GLIMPSE source name
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col2" datatype="float" name="GLON" precision="4" ucd="pos.galactic.lon" unit="deg" width="8">
    <DESCRIPTION>
     Galactic longtitude (1) These coordinates are set to the average
     position of the source at            4.5 and at 8.0 microns. This
     position may differ slightly from the            `official'
     GLIMPSE position in cases where PSF fitting was used to
     determine the flux of the source if the position of the source
     was            adjusted to obtain a better residual.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col3" datatype="float" name="GLAT" precision="4" ucd="pos.galactic.lat" unit="deg" width="7">
    <DESCRIPTION>
     Galactic latitude (1) These coordinates are set to the average
     position of the source at            4.5 and at 8.0 microns. This
     position may differ slightly from the            `official'
     GLIMPSE position in cases where PSF fitting was used to
     determine the flux of the source if the position of the source
     was            adjusted to obtain a better residual.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col4" datatype="float" name="RAdeg" precision="4" ucd="pos.eq.ra" unit="deg" width="8">
    <DESCRIPTION>
     Right Ascension in decimal degrees (J2000) (1) These coordinates
     are set to the average position of the source at            4.5
     and at 8.0 microns. This position may differ slightly from the
     `official' GLIMPSE position in cases where PSF fitting was used
     to            determine the flux of the source if the position of
     the source was            adjusted to obtain a better residual.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col5" datatype="float" name="DEdeg" precision="4" ucd="pos.eq.dec" unit="deg" width="8">
    <DESCRIPTION>
     Declination in decimal degrees (J2000) (1) These coordinates are
     set to the average position of the source at            4.5 and
     at 8.0 microns. This position may differ slightly from the
     `official' GLIMPSE position in cases where PSF fitting was used
     to            determine the flux of the source if the position of
     the source was            adjusted to obtain a better residual.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col6" datatype="float" name="Jmag" precision="2" ucd="phot.mag;em.IR.J" unit="mag" width="5">
    <DESCRIPTION>
     ? 2MASS J band magnitude (2) The zero-magnitude fluxes assumed
     throughout this paper are:            F_{nu}_(J) = 1594 Jy,
     F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col7" datatype="float" name="Hmag" precision="2" ucd="phot.mag;em.IR.H" unit="mag" width="5">
    <DESCRIPTION>
     ? 2MASS H band magnitude (2) The zero-magnitude fluxes assumed
     throughout this paper are:            F_{nu}_(J) = 1594 Jy,
     F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col8" datatype="float" name="Kmag" precision="2" ucd="phot.mag;em.IR.K" unit="mag" width="5">
    <DESCRIPTION>
     ? 2MASS K_s_ band magnitude (2) The zero-magnitude fluxes assumed
     throughout this paper are:            F_{nu}_(J) = 1594 Jy,
     F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col9" datatype="float" name="G3.6mag" precision="2" ucd="phot.mag;em.IR.3-4um" unit="mag" width="5">
    <DESCRIPTION>
     ? GLIMPSE catalog 3.6 micron band magnitude (2) The zero-
     magnitude fluxes assumed throughout this paper are:
     F_{nu}_(J) = 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7
     Jy,           F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5
     microns) = 179.7 Jy,            F_{nu}_(5.8 microns) = 115.0 Jy,
     F_{nu}_(8.0 microns) = 64.13 Jy,            F_{nu}_(MSX E) = 8.75
     Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col10" datatype="float" name="G4.5mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="5">
    <DESCRIPTION>
     GLIMPSE catalog 4.5 micron band magnitude (2) The zero-magnitude
     fluxes assumed throughout this paper are:            F_{nu}_(J) =
     1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col11" datatype="float" name="G5.8mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="5">
    <DESCRIPTION>
     ? GLIMPSE catalog 5.8 micron band magnitude (2) The zero-
     magnitude fluxes assumed throughout this paper are:
     F_{nu}_(J) = 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7
     Jy,           F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5
     microns) = 179.7 Jy,            F_{nu}_(5.8 microns) = 115.0 Jy,
     F_{nu}_(8.0 microns) = 64.13 Jy,            F_{nu}_(MSX E) = 8.75
     Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col12" datatype="float" name="G8.0mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="4">
    <DESCRIPTION>
     GLIMPSE catalog 8.0 micron band magnitude (2) The zero-magnitude
     fluxes assumed throughout this paper are:            F_{nu}_(J) =
     1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col13" datatype="float" name="4.5mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="5">
    <DESCRIPTION>
     This paper's 4.5 micron band magnitude (2) The zero-magnitude
     fluxes assumed throughout this paper are:            F_{nu}_(J) =
     1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col14" datatype="float" name="8.0mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="4">
    <DESCRIPTION>
     This paper's 8.0 micron band magnitude (2) The zero-magnitude
     fluxes assumed throughout this paper are:            F_{nu}_(J) =
     1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col15" datatype="float" name="Emag" precision="2" ucd="phot.mag;em.IR.8-15um" unit="mag" width="5">
    <DESCRIPTION>
     ? This paper's MSX E band magnitude (2) The zero-magnitude fluxes
     assumed throughout this paper are:            F_{nu}_(J) = 1594
     Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col16" datatype="float" name="24mag" precision="2" ucd="phot.mag;em.IR.15-30um" unit="mag" width="4">
    <DESCRIPTION>
     ? This paper's 24 micron band magnitude (2) The zero-magnitude
     fluxes assumed throughout this paper are:            F_{nu}_(J) =
     1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy,
     F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy,
     F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy,
     F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy.
    </DESCRIPTION>
   </FIELD>
   <FIELD ID="col17" arraysize="2" datatype="char" name="f_Name" ucd="meta.code" unit="---">
    <DESCRIPTION>
     Flag on Name (3)  This column lists two characters, which are
     flags for 4.5 and            8.0 microns respectively.      A =
     GLIMPSE Catalog magnitudes are in agreement with the independent
     magnitudes calculated in this paper;     I = the independent
     magnitudes calculated in this paper should be trusted
     over the GLIMPSE Catalog magnitudes.
    </DESCRIPTION>
   </FIELD>
   <DATA>
    <TABLEDATA>
     <TR>
      <TD>SSTGLMC G000.0000+00.1611</TD>
      <TD>  0.0000</TD>
      <TD> 0.1611</TD>
      <TD>266.2480</TD>
      <TD>-28.8521</TD>
      <TD/>
      <TD/>
      <TD/>
      <TD> 9.78</TD>
      <TD> 9.19</TD>
      <TD> 8.64</TD>
      <TD>8.05</TD>
      <TD> 9.13</TD>
      <TD>8.17</TD>
      <TD/>
      <TD/>
      <TD>AA</TD>
     </TR>
    </TABLEDATA>
   </DATA>
  </TABLE>
 </RESOURCE>
</VOTABLE>
